Why Is the Cosmic Microwave Background Fluctuation Level 10−5?

Tegmark, Max, Rees, Martin J.·1998·The Astrophysical Journal

Cited by (159)

Items 101–159 of 159

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  10. Signals of Inflation in a Friendly String Landscape
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    Molly E. C. Swanson · 2008 · arXiv (Cornell University)
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